Zobrazeno 1 - 10
of 118
pro vyhledávání: '"Mccrum, M."'
Autor:
McCrum, M. G. I.
The focus of this thesis is the study of superluminous supernovae (SLSNe) within the Pan- STARRSI Medium Deep Survey (PSI MDS). Previous work on SLSNe has displayed a trend in their host environments, in that they seem to preferentially occur in low
Externí odkaz:
http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.679257
Autor:
Scolnic, D. M., Jones, D. O., Rest, A., Pan, Y. C., Chornock, R., Foley, R. J., Huber, M. E., Kessler, R., Narayan, G., Riess, A. G., Rodney, S., Berger, E., Brout, D. J., Challis, P. J., Drout, M., Finkbeiner, D., Lunnan, R., Kirshner, R. P., Sanders, N. E., Schlafly, E., Smartt, S., Stubbs, C. W., Tonry, J., Wood-Vasey, W. M., Foley, M., Hand, J., Johnson, E., Burgett, W. S., Chambers, K. C., Draper, P. W., Hodapp, K. W., Kaiser, N., Kudritzki, R. P., Magnier, E. A., Metcalfe, N., Bresolin, F., Gall, E., Kotak, R., McCrum, M., Smith, K. W.
We present optical light curves, redshifts, and classifications for 365 spectroscopically confirmed Type Ia supernovae (SNe Ia) discovered by the Pan-STARRS1 (PS1) Medium Deep Survey. We detail improvements to the PS1 SN photometry, astrometry and ca
Externí odkaz:
http://arxiv.org/abs/1710.00845
Autor:
Jones, D. O., Scolnic, D. M., Riess, A. G., Rest, A., Kirshner, R. P., Berger, E., Kessler, R., Pan, Y. -C., Foley, R. J., Chornock, R., Ortega, C. A., Challis, P. J., Burgett, W. S., Chambers, K. C., Draper, P. W., Flewelling, H., Huber, M. E., Kaiser, N., Kudritzki, R. -P., Metcalfe, N., Tonry, J., Wainscoat, R. J., Waters, C., Gall, E. E. E., Kotak, R., McCrum, M., Smartt, S. J., Smith, K. W.
We use 1169 Pan-STARRS supernovae (SNe) and 195 low-$z$ ($z < 0.1$) SNe Ia to measure cosmological parameters. Though most Pan-STARRS SNe lack spectroscopic classifications, in a previous paper (I) we demonstrated that photometrically classified SNe
Externí odkaz:
http://arxiv.org/abs/1710.00846
Autor:
Inserra, C., Fraser, M., Smartt, S. J., Benetti, S., Chen, T. -W., Childress, M., Gal-Yam, A., Howell, D. A., Kangas, T., Pignata, G., Polshaw, J., Sullivan, M., Smith, K. W., Valenti, S., Young, D. R., Parker, S., Seccull, T., McCrum, M.
We present the complete set of ultra-violet, optical and near-infrared photometry and spectroscopy for SN 2012ca, covering the period from 6~days prior to maximum light, until 531 days after maximum. The spectroscopic time series for SN 2012ca is ess
Externí odkaz:
http://arxiv.org/abs/1510.01109
Autor:
Lunnan, R., Chornock, R., Berger, E., Rest, A., Fong, W., Scolnic, D., Jones, D., Soderberg, A. M., Challis, P. M., Drout, M. R., Foley, R. J., Huber, M. E., Kirshner, R. P., Leibler, C., Marion, G. H., McCrum, M., Milisavljevic, D., Narayan, G., Sanders, N. E., Smartt, S. J., Smith, K. W., Tonry, J. L., Burgett, W. S., Chambers, K. C., Flewelling, H., Kudritzki, R. -P., Wainscoat, R. J., Waters, C.
Publikováno v:
ApJ, 804, 90 (2015)
We present Hubble Space Telescope (HST) rest-frame ultraviolet imaging of the host galaxies of 16 hydrogen-poor superluminous supernovae (SLSNe), including 11 events from the Pan-STARRS Medium Deep Survey. Taking advantage of the superb angular resol
Externí odkaz:
http://arxiv.org/abs/1411.1060
Autor:
Smartt, S. J., Valenti, S., Fraser, M., Inserra, C., Young, D. R., Sullivan, M., Pastorello, A., Benetti, S., Gal-Yam, A., Knapic, C., Molinaro, M., Smareglia, R., Smith, K. W., Taubenberger, S., Yaron, O., Anderson, J. P., Ashall, C., Balland, C., Baltay, C., Barbarino, C., Bauer, F. E., Baumont, S., Bersier, D., Blagorodnova, N., Bongard, S., Botticella, M. T., Bufano, F., Bulla, M., Cappellaro, E., Campbell, H., Cellier-Holzem, F., Chen, T. -W., Childress, M. J., Clocchiatti, A., Contreras, C., Ora, M. Dall, Danziger, J., de Jaeger, T., De Cia, A., Della Valle, M., Dennefeld, M., Elias-Rosa, N., Elman, N., Feindt, U., Fleury, M., Gall, E., Gonzalez-Gaitan, S., Galbany, L., Garoffolo, A. Morales, Greggio, L., Guillou, L. L., Hachinger, S., Hadjiyska, E., Hage, P. E., Hillebrandt, W., Hodgkin, S., Hsiao, E. Y., James, P. A., Jerkstrand, A., Kangas, T., Kankare, E., Kotak, R., Kromer, M., Kuncarayakti, H., Leloudas, G., Lundqvist, P., Lyman, J. D., Hook, I. M., Maguire, K., Manulis, I., Margheim, S. J., Mattila, S., Maund, J. R., Mazzali, P. A., McCrum, M., McKinnon, R., Moreno-Raya, M. E., Nicholl, M., Nugent, P., Pain, R., Phillips, M. M., Pignata, G., Polshaw, J., Pumo, M. L., Rabinowitz, D., Reilly, E., Romero-Canizales, C., Scalzo, R., Schmidt, B., Schulze, S., Sim, S., Sollerman, J., Taddia, F., Tartaglia, L., Terreran, G., Tomasella, L., Turatto, M., Walker, E., Walton, N. A., Wyrzykowski, L., Yuan, F., Zampieri, L.
Publikováno v:
A&A 579, A40 (2015)
The Public European Southern Observatory Spectroscopic Survey of Transient Objects (PESSTO) began as a public spectroscopic survey in April 2012. We describe the data reduction strategy and data products which are publicly available through the ESO a
Externí odkaz:
http://arxiv.org/abs/1411.0299
Autor:
Nicholl, M., Smartt, S. J., Jerkstrand, A., Inserra, C., Anderson, J. P., Baltay, C., Benetti, S., Chen, T. -W., Elias-Rosa, N., Feindt, U., Fraser, M., Gal-Yam, A., Hadjiyska, E., Howell, D. A., Kotak, R., Lawrence, A., Leloudas, G., Margheim, S., Mattila, S., McKinnon, R., McCrum, M., Mead, A., Nugent, P., Rabinowitz, D., Rest, A., Smith, K. W., Sollerman, J., Sullivan, M., Taddia, F., Valenti, S., Walker, E. S., Young, D. R.
Publikováno v:
2014, MNRAS, 444, 2096
We present optical spectra and light curves for three hydrogen-poor super-luminous supernovae followed by the Public ESO Spectroscopic Survey of Transient Objects (PESSTO). Time series spectroscopy from a few days after maximum light to 100 days late
Externí odkaz:
http://arxiv.org/abs/1405.1325
Autor:
McCrum, M., Smartt, S. J., Rest, A., Smith, K., Kotak, R., Rodney, S. A., Young, D. R., Chornock, R., Berger, E., Foley, R. J., Fraser, M., Wright, D., Scolnic, D., Tonry, J. L., Urata, Y., Huang, K., Pastorello, A., Botticella, M. T., Valenti, S., Mattila, S., Kankare, E., Farrow, D. J., Huber, M. E., Stubbs, C. W., Kirshner, R. P., Bresolin, F., Burgett, W. S., Chambers, K. C., Draper, P. W., Flewelling, H., Jedicke, R., Kaiser, N., Magnier, E. A., Metcalfe, N., Morgan, J. S., Price, P. A., Sweeney, W., Wainscoat, R. J., Waters, C.
The Pan-STARRS1 (PS1) survey has obtained imaging in 5 bands (grizy_P1) over 10 Medium Deep Survey (MDS) fields covering a total of 70 square degrees. This paper describes the search for apparently hostless supernovae (SNe) within the first year of P
Externí odkaz:
http://arxiv.org/abs/1402.1631
Hydrogen-Poor Superluminous Supernovae and Long-Duration Gamma-Ray Bursts Have Similar Host Galaxies
Autor:
Lunnan, R., Chornock, R., Berger, E., Laskar, T., Fong, W., Rest, A., Sanders, N. E., Challis, P. M., Drout, M. R., Foley, R. J., Huber, M. E., Kirshner, R. P., Leibler, C., Marion, G. H., McCrum, M., Milisavljevic, D., Narayan, G., Scolnic, D., Smartt, S. J., Smith, K. W., Soderberg, A. M., Tonry, J. L., Burgett, W. S., Chambers, K. C., Flewelling, H., Hodapp, K. W., Kaiser, N., Magnier, E. A., Price, P. A., Wainscoat, R. J.
Publikováno v:
Astrophys.J. 787:138-156 (2014)
We present optical spectroscopy and optical/near-IR photometry of 31 host galaxies of hydrogen-poor superluminous supernovae (SLSNe), including 15 events from the Pan-STARRS1 Medium Deep Survey. Our sample spans the redshift range 0.1 < z < 1.6 and i
Externí odkaz:
http://arxiv.org/abs/1311.0026
Autor:
McCrum, M., Smartt, S. J., Kotak, R., Rest, A., Jerkstrand, A., Inserra, C., Rodney, S. A., Chen, T. -W., Howell, D. A., Huber, M. E., Pastorello, A., Tonry, J. L., Bresolin, F., Kudritzki, R. -P., Chornock, R., Berger, E., Smith, K., Botticella, M. T., Foley, R. J., Fraser, M., Milisavljevic, D., Nicholl, M., Riess, A. G., Stubbs, C. W., Valenti, S., Wood-Vasey, W. M., Wright, D., Young, D. R., Drout, M., Czekala, I., Burgett, W. S., Chambers, K. C., Draper, P., Flewelling, H., Hodapp, K. W., Kaiser, N., Magnier, E. A., Metcalfe, N., Sweeney, W., Wainscoat, R. J.
We present optical photometric and spectroscopic coverage of the superluminous supernova (SLSN) PS1-11ap, discovered with the Pan-STARRS1 Medium Deep Survey at z = 0.524. This intrinsically blue transient rose slowly to reach a peak magnitude of M_u
Externí odkaz:
http://arxiv.org/abs/1310.4417